! Started logfile: J0539+1433_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:15:06 2011
obs J0539+1433_X_2010_10_13_pus_uva.fits
! Reading UV FITS file: J0539+1433_X_2010_10_13_pus_uva.fits
! AN table 1: 135 integrations on 105 of 105 possible baselines.
! AN table 2: 21 integrations on 105 of 105 possible baselines.
! AN table 3: 167 integrations on 105 of 105 possible baselines.
! Apparent sampling: 0.158455 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0539+1433
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.40996e+09        8e+06          1        8e+06
!  02        2  8.47996e+09        8e+06          1        8e+06
!  03        3  8.79496e+09        8e+06          1        8e+06
!  04        4  8.89996e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 5978 lines of history.
! 
! Reading 21496 visibilities.
select I
! Polarization I is unavailable.
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
print "field_size =",field_size
! field_size = 256 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J0539+1433_X_2010_10_13_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 1356 telescope corrections were flagged in sub-array 1.
!  A total of 236 telescope corrections were flagged in sub-array 2.
!  A total of 1780 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1356 telescope corrections were flagged in sub-array 1.
!  A total of 236 telescope corrections were flagged in sub-array 2.
!  A total of 1780 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1356 telescope corrections were flagged in sub-array 1.
!  A total of 236 telescope corrections were flagged in sub-array 2.
!  A total of 1780 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1356 telescope corrections were flagged in sub-array 1.
!  A total of 236 telescope corrections were flagged in sub-array 2.
!  A total of 1780 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.673515Jy  sigma=0.007329
! Fit after  self-cal, rms=0.629787Jy  sigma=0.006934
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 10.4% of the data.
!  The x-axis pixel size should ideally be below 0.1558 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.5649 mas, bmaj=1.019 mas, bpa=0.5263 degrees
! Estimated noise=739.178 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.298786 Jy
! Component: 100  -  total flux cleaned = 0.368273 Jy
! Total flux subtracted in 100 components = 0.368273 Jy
! Clean residual min=-0.010352 max=0.027373 Jy/beam
! Clean residual mean=0.000387 rms=0.003370 Jy/beam
! Combined flux in latest and established models = 0.368273 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.368273 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.173393Jy  sigma=0.001579
! Fit after  self-cal, rms=0.173445Jy  sigma=0.001578
! Inverting map 
! Your choice of large map pixels excluded 10.4% of the data.
!  The x-axis pixel size should ideally be below 0.1558 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0319303 Jy
! Component: 100  -  total flux cleaned = 0.0513734 Jy
! Total flux subtracted in 100 components = 0.0513734 Jy
! Clean residual min=-0.007935 max=0.011904 Jy/beam
! Clean residual mean=0.000193 rms=0.002391 Jy/beam
! Combined flux in latest and established models = 0.419646 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 19 components and 0.419646 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.165255Jy  sigma=0.001423
! Fit after  self-cal, rms=0.165277Jy  sigma=0.001423
! Inverting map 
! Your choice of large map pixels excluded 10.4% of the data.
!  The x-axis pixel size should ideally be below 0.1558 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 10.4% of the data.
!  The x-axis pixel size should ideally be below 0.1558 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7349 mas, bmaj=1.347 mas, bpa=-1.493 degrees
! Estimated noise=466.016 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0.2, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0237435 Jy
! Component: 100  -  total flux cleaned = 0.0363596 Jy
! Component: 150  -  total flux cleaned = 0.0440485 Jy
! Component: 200  -  total flux cleaned = 0.0491097 Jy
! Total flux subtracted in 200 components = 0.0491097 Jy
! Clean residual min=-0.005048 max=0.006401 Jy/beam
! Clean residual mean=0.000002 rms=0.001550 Jy/beam
! Combined flux in latest and established models = 0.468756 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 38 components and 0.468756 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162911Jy  sigma=0.001369
! Fit after  self-cal, rms=0.162807Jy  sigma=0.001368
! Inverting map 
! Your choice of large map pixels excluded 10.4% of the data.
!  The x-axis pixel size should ideally be below 0.1558 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.84     HH        1.06     HN        1.05     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        1.00     
!   MK        1.00*    NL        1.01     NY        1.01     OV        1.00     
!   PT        0.96     SC        0.99     TS        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        0.84     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        0.97     LA        0.99     
!   MK        1.00*    NL        1.00*    NY        1.04     OV        0.97     
!   PT        0.98     SC        1.00*    TS        1.00*    
! 
!  A total of 75 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        0.81     HH        1.16     HN        1.09     
!   KB        1.01     KK        0.89     KP        1.00     LA        1.00     
!   MK        1.02     NL        0.99     NY        1.02     OV        0.98     
!   PT        0.95     SC        1.00     TS        1.05     
! 
! 
! Correcting IF 2.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        0.99     HH        0.99     HN        1.10     
!   KB        1.00*    KK        1.00*    KP        1.00     LA        0.94     
!   MK        1.00*    NL        1.03     NY        1.05     OV        1.01     
!   PT        1.00     SC        1.00     TS        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.97     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        0.97     LA        0.98     
!   MK        1.00*    NL        1.00*    NY        1.06     OV        0.98     
!   PT        0.95     SC        1.00*    TS        1.00*    
! 
!  A total of 75 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        0.96     HH        1.06     HN        1.05     
!   KB        1.01     KK        0.96     KP        0.99     LA        0.95     
!   MK        0.95     NL        1.03     NY        0.98     OV        1.00     
!   PT        0.97     SC        1.02     TS        1.13     
! 
! 
! Correcting IF 3.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.00     HH        1.01     HN        1.09     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        0.94     
!   MK        1.00*    NL        1.01     NY        1.08     OV        0.98     
!   PT        1.02     SC        1.01     TS        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.98     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        0.99     LA        0.97     
!   MK        1.00*    NL        1.00*    NY        1.07     OV        0.99     
!   PT        1.04     SC        1.00*    TS        1.00*    
! 
!  A total of 75 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        0.98     HH        1.11     HN        1.07     
!   KB        1.01     KK        0.93     KP        0.99     LA        0.95     
!   MK        1.00     NL        0.98     NY        1.10     OV        0.99     
!   PT        1.00     SC        1.07     TS        1.03     
! 
! 
! Correcting IF 4.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.00     HH        0.94     HN        1.09     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        1.01     
!   MK        1.00*    NL        1.02     NY        1.04     OV        1.03     
!   PT        0.99     SC        0.99     TS        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.05     FD        0.98     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        1.02     LA        1.03     
!   MK        1.00*    NL        1.00*    NY        0.97     OV        1.04     
!   PT        0.93     SC        1.00*    TS        1.00*    
! 
!  A total of 75 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.06     FD        0.98     HH        1.08     HN        0.97     
!   KB        1.01     KK        1.00     KP        1.02     LA        1.03     
!   MK        0.99     NL        1.02     NY        1.11     OV        1.02     
!   PT        0.98     SC        1.01     TS        0.91     
! 
! 
! Fit before self-cal, rms=0.162807Jy  sigma=0.001368
! Fit after  self-cal, rms=0.162569Jy  sigma=0.001341
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7402 mas, bmaj=1.372 mas, bpa=-2.163 degrees
! Estimated noise=467.341 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00151629 Jy
! Component: 100  -  total flux cleaned = -0.00242328 Jy
! Component: 150  -  total flux cleaned = -0.00288793 Jy
! Component: 200  -  total flux cleaned = -0.00320178 Jy
! Total flux subtracted in 200 components = -0.00320178 Jy
! Clean residual min=-0.005415 max=0.004363 Jy/beam
! Clean residual mean=-0.000011 rms=0.001293 Jy/beam
! Combined flux in latest and established models = 0.465554 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 48 components and 0.465554 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162434Jy  sigma=0.001340
! Fit after  self-cal, rms=0.162501Jy  sigma=0.001340
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162501Jy  sigma=0.001340
! Fit after  self-cal, rms=0.161361Jy  sigma=0.001314
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7401 mas, bmaj=1.383 mas, bpa=-2.594 degrees
! Estimated noise=467.15 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000781021 Jy
! Component: 100  -  total flux cleaned = 0.000734165 Jy
! Component: 150  -  total flux cleaned = 0.000733619 Jy
! Component: 200  -  total flux cleaned = 0.000690097 Jy
! Total flux subtracted in 200 components = 0.000690097 Jy
! Clean residual min=-0.003160 max=0.003072 Jy/beam
! Clean residual mean=-0.000033 rms=0.000838 Jy/beam
! Combined flux in latest and established models = 0.466244 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 61 components and 0.466244 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.161328Jy  sigma=0.001314
! Fit after  self-cal, rms=0.161434Jy  sigma=0.001313
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -7.74827e-05 Jy
! Component: 100  -  total flux cleaned = -7.74021e-05 Jy
! Component: 150  -  total flux cleaned = -0.000113043 Jy
! Component: 200  -  total flux cleaned = -0.000144435 Jy
! Total flux subtracted in 200 components = -0.000144435 Jy
! Clean residual min=-0.003069 max=0.003081 Jy/beam
! Clean residual mean=-0.000032 rms=0.000846 Jy/beam
! Combined flux in latest and established models = 0.4661 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 66 components and 0.4661 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.161412Jy  sigma=0.001313
! Fit after  self-cal, rms=0.161405Jy  sigma=0.001313
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.161405Jy  sigma=0.001313
! Fit after  self-cal, rms=0.172619Jy  sigma=0.001306
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7422 mas, bmaj=1.394 mas, bpa=-2.94 degrees
! Estimated noise=467.977 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 4.32655e-05 Jy
! Component: 100  -  total flux cleaned = 4.23508e-05 Jy
! Component: 150  -  total flux cleaned = 9.20577e-05 Jy
! Component: 200  -  total flux cleaned = 0.000137673 Jy
! Total flux subtracted in 200 components = 0.000137673 Jy
! Clean residual min=-0.002231 max=0.002656 Jy/beam
! Clean residual mean=0.000003 rms=0.000628 Jy/beam
! Combined flux in latest and established models = 0.466238 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 70 components and 0.466238 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172574Jy  sigma=0.001305
! Fit after  self-cal, rms=0.173130Jy  sigma=0.001305
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 5.77723e-05 Jy
! Component: 100  -  total flux cleaned = 9.9869e-05 Jy
! Component: 150  -  total flux cleaned = 9.94019e-05 Jy
! Component: 200  -  total flux cleaned = 9.89833e-05 Jy
! Total flux subtracted in 200 components = 9.89833e-05 Jy
! Clean residual min=-0.002265 max=0.002636 Jy/beam
! Clean residual mean=0.000001 rms=0.000622 Jy/beam
! Combined flux in latest and established models = 0.466337 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 73 components and 0.466337 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.173105Jy  sigma=0.001304
! Fit after  self-cal, rms=0.173104Jy  sigma=0.001304
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.173104Jy  sigma=0.001304
! Fit after  self-cal, rms=0.175551Jy  sigma=0.001304
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=2.667 mas, bmaj=2.88 mas, bpa=-14.79 degrees
! Estimated noise=579.936 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000221355 Jy
! Component: 100  -  total flux cleaned = 0.000152569 Jy
! Component: 150  -  total flux cleaned = 0.000126062 Jy
! Component: 200  -  total flux cleaned = 0.000106446 Jy
! Total flux subtracted in 200 components = 0.000106446 Jy
! Clean residual min=-0.001984 max=0.002547 Jy/beam
! Clean residual mean=-0.000006 rms=0.000688 Jy/beam
! Combined flux in latest and established models = 0.466443 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 76 components and 0.466443 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.175554Jy  sigma=0.001304
! Fit after  self-cal, rms=0.175646Jy  sigma=0.001304
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00013571 Jy
! Component: 100  -  total flux cleaned = 0.000135119 Jy
! Component: 150  -  total flux cleaned = 0.000117412 Jy
! Component: 200  -  total flux cleaned = 0.000117639 Jy
! Total flux subtracted in 200 components = 0.000117639 Jy
! Clean residual min=-0.001963 max=0.002533 Jy/beam
! Clean residual mean=-0.000012 rms=0.000690 Jy/beam
! Combined flux in latest and established models = 0.466561 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 77 components and 0.466561 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.175650Jy  sigma=0.001304
! Fit after  self-cal, rms=0.175658Jy  sigma=0.001304
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7429 mas, bmaj=1.394 mas, bpa=-2.967 degrees
! Estimated noise=467.818 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7429 x 1.394 at -2.967 degrees (North through East)
! Clean map  min=-0.0019188  max=0.39835 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  flux_cutoff = imstat(rms) * dynam
  repeat
    if (peak(flux) > flux_cutoff) peakwin win_mult
    clean clean_niter,clean_gain
    flux_cutoff = imstat(rms) * dynam
    selfcal
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.5683 mas, bmaj=1.05 mas, bpa=-1.066 degrees
! Estimated noise=747.851 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.300575 Jy
! Component: 100  -  total flux cleaned = 0.369432 Jy
! Component: 150  -  total flux cleaned = 0.39966 Jy
! Component: 200  -  total flux cleaned = 0.417788 Jy
! Total flux subtracted in 200 components = 0.417788 Jy
! Clean residual min=-0.004837 max=0.009723 Jy/beam
! Clean residual mean=0.000177 rms=0.001445 Jy/beam
! Combined flux in latest and established models = 0.417788 Jy
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 23 model components to the UV plane model.
! The established model now contains 23 components and 0.417788 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7429 mas, bmaj=1.394 mas, bpa=-2.967 degrees
! Estimated noise=467.818 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.020978 Jy
! Component: 100  -  total flux cleaned = 0.0318873 Jy
! Component: 150  -  total flux cleaned = 0.038267 Jy
! Component: 200  -  total flux cleaned = 0.0421409 Jy
! Total flux subtracted in 200 components = 0.0421409 Jy
! Clean residual min=-0.002181 max=0.002882 Jy/beam
! Clean residual mean=0.000089 rms=0.000694 Jy/beam
! Combined flux in latest and established models = 0.459929 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 42 components and 0.459929 Jy
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=2.667 mas, bmaj=2.88 mas, bpa=-14.79 degrees
! Estimated noise=579.936 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00370856 Jy
! Component: 100  -  total flux cleaned = 0.0052724 Jy
! Component: 150  -  total flux cleaned = 0.00596889 Jy
! Component: 200  -  total flux cleaned = 0.00611116 Jy
! Total flux subtracted in 200 components = 0.00611116 Jy
! Clean residual min=-0.002005 max=0.002498 Jy/beam
! Clean residual mean=0.000005 rms=0.000674 Jy/beam
! Combined flux in latest and established models = 0.466041 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.49916e-05 Jy
! Component: 100  -  total flux cleaned = 7.04188e-05 Jy
! Component: 150  -  total flux cleaned = 9.11152e-05 Jy
! Component: 200  -  total flux cleaned = 0.000111378 Jy
! Total flux subtracted in 200 components = 0.000111378 Jy
! Clean residual min=-0.002006 max=0.002502 Jy/beam
! Clean residual mean=0.000001 rms=0.000671 Jy/beam
! Combined flux in latest and established models = 0.466152 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 57 components and 0.466152 Jy
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! Estimated beam: bmin=0.7429 mas, bmaj=1.394 mas, bpa=-2.967 degrees
! Estimated noise=467.818 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000671844 Jy
! Component: 100  -  total flux cleaned = -0.000672958 Jy
! Component: 150  -  total flux cleaned = -0.000672513 Jy
! Component: 200  -  total flux cleaned = -0.000638395 Jy
! Total flux subtracted in 200 components = -0.000638395 Jy
! Clean residual min=-0.001951 max=0.002546 Jy/beam
! Clean residual mean=0.000012 rms=0.000593 Jy/beam
! Combined flux in latest and established models = 0.465513 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 64 components and 0.465514 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.175685Jy  sigma=0.001305
! Fit after  self-cal, rms=0.175732Jy  sigma=0.001304
wmodel J0539+1433_X_2010_10_13_pus_map.mod
! Writing 64 model components to file: J0539+1433_X_2010_10_13_pus_map.mod
wobs J0539+1433_X_2010_10_13_pus_uvs.fits
! Writing UV FITS file: J0539+1433_X_2010_10_13_pus_uvs.fits
wwins J0539+1433_X_2010_10_13_pus_map.win
! wwins: Wrote 2 windows to J0539+1433_X_2010_10_13_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000547719 Jy
! Component: 100  -  total flux cleaned = 0.000438818 Jy
! Component: 150  -  total flux cleaned = 0.000506369 Jy
! Component: 200  -  total flux cleaned = 0.000572089 Jy
! Component: 250  -  total flux cleaned = 0.000730039 Jy
! Component: 300  -  total flux cleaned = 0.000760312 Jy
! Component: 350  -  total flux cleaned = 0.000850004 Jy
! Component: 400  -  total flux cleaned = 0.000790984 Jy
! Component: 450  -  total flux cleaned = 0.000819608 Jy
! Component: 500  -  total flux cleaned = 0.000904145 Jy
! Component: 550  -  total flux cleaned = 0.000903713 Jy
! Component: 600  -  total flux cleaned = 0.000930785 Jy
! Component: 650  -  total flux cleaned = 0.00098478 Jy
! Component: 700  -  total flux cleaned = 0.00109104 Jy
! Component: 750  -  total flux cleaned = 0.0011173 Jy
! Component: 800  -  total flux cleaned = 0.00116893 Jy
! Component: 850  -  total flux cleaned = 0.00119441 Jy
! Component: 900  -  total flux cleaned = 0.00124502 Jy
! Component: 950  -  total flux cleaned = 0.00127 Jy
! Component: 1000  -  total flux cleaned = 0.00139397 Jy
! Total flux subtracted in 1024 components = 0.00136939 Jy
! Clean residual min=-0.001452 max=0.001734 Jy/beam
! Clean residual mean=0.000008 rms=0.000491 Jy/beam
! Combined flux in latest and established models = 0.466883 Jy
keep
! Adding 73 model components to the UV plane model.
! The established model now contains 137 components and 0.466883 Jy
![Exited script file: muppet]
wmap "J0539+1433_X_2010_10_13_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7429 x 1.394 at -2.967 degrees (North through East)
! Clean map  min=-0.0016518  max=0.39931 Jy/beam
! Writing clean map to FITS file: J0539+1433_X_2010_10_13_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.399315 
invert
! Inverting map 
! Your choice of large map pixels excluded 10.1% of the data.
!  The x-axis pixel size should ideally be below 0.1559 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1748 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00048985 
device "J0539+1433_X_2010_10_13_pus\_map.eps/VPS"
! Attempting to open device: 'J0539+1433_X_2010_10_13_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.368018 0.368018 0.736036 1.47207 2.94414 5.88829 11.7766 23.5532 47.1063 94.2126
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.399 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7429 x 1.394 at -2.967 degrees (North through East)
! Clean map  min=-0.0016518  max=0.39931 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0539+1433_X_2010_10_13_pus\_map.gif/vgif"
! Attempting to open device: 'J0539+1433_X_2010_10_13_pus_map.gif/vgif'
mapplot cln